Lecture- Tutorials for Introductory Astronomy
3rd Edition
ISBN: 9780321820464
Author: Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher: Addison-Wesley
expand_more
expand_more
format_list_bulleted
Textbook Question
Chapter 2, Problem 3KESP
Draw two lines: one connecting the planet at Position A to the star and a second line connecting the planet at Position B to the star. Shade in the area swept out by the planet when traveling from Positions A to B.
Expert Solution & Answer
Learn your wayIncludes step-by-step video
schedule02:10
Students have asked these similar questions
The intensity of light from a central source varies inversely as the square of the distance. If you lived on a planet only half as far from the Sun as our Earth, how would Sun’s light intensity compare with that on Earth? How about a planet 10 times farther away than Earth?
1- MODIS is an Earth Observation sensor onboard TERRA spacecraft flying in a near-polar circular orbit with an orbital period of 98.8 minutes. The width of the swath imaged by MODIS is 2330 km.
A- How many orbits does TERRA trace in one day?
B- Assuming that the Earth rotates around its polar axis at a rate of 0.2618 rd/hr and that the equatorial radius is 6378 km, do two consecutive swaths of MODIS overlap at the equator? (hint: the length of an arc = angle in rd * radius)
C- The radius of the latitude circle at 35 deg is 5224.5 km. Do two consecutive swaths of MODIS overlap at latitude 35 deg?
2- An aerostationary orbit for Mars is equivalent to a geostationary orbit for Earth. It is designed to enable a satellite in that orbit to image always the same surface of Mars. Calculate the altitude of an aerostationary orbit assuming that Mars is spherical, that its sidereal rotational period is 1.02595676 Earth days, its equatorial radius is 3389.50 km and its mass is…
Mercury's orbit ranges from 46 to 70 million km from the Sun, while Earth orbits at about 150 million km.
a. The Sun has a 30-arc-minute diameter viewed from Earth; what range of sizes does it have when viewed from Mercury?
When Mercury is 46 million km from the Sun, the Sun has a diameter of
When Mercury is 70 million km from the Sun, the Sun has a diameter of
arc-minutes.
arc-minutes.
b. At Mercury's orbital extremes, how many times stronger is the Sun's radiation on Mercury than on Earth?
At 46 million km, the Sun's radiation is
times stronger than on Earth.
At 70 million km, the Sun's radiation is
times stronger than on Earth.
Chapter 2 Solutions
Lecture- Tutorials for Introductory Astronomy
Ch. 2 - Does this planet obey Kepler's second law? How do...Ch. 2 - If you were carefully watching this planet during...Ch. 2 - Draw two lines: one connecting the planet at...Ch. 2 - Pick any two planet positions (C, D, E, F, G, H,...Ch. 2 - How would the time it takes the planet to travel...Ch. 2 - During which of the two time intervals for which...Ch. 2 - During which of the two time intervals for which...Ch. 2 - Does the planet appear to be traveling the same...Ch. 2 - At which position would the planet have been...Ch. 2 - At Position D, is the speed of the planet...
Ch. 2 - Provide a concise statement that describes the...Ch. 2 - Which of the three orbits shown below (A, B, or C)...Ch. 2 - Which of the listed objects would experience the...Ch. 2 - Describe the extent to which you think Earth's...Ch. 2 - Which of the two planets (Esus or Sulis) do you...Ch. 2 - If Esus and Sulis were to switch positions, would...Ch. 2 - Do you think the orbital period for Esus would...Ch. 2 - Imagine both Esus and Sulis were in orbit around...Ch. 2 - According to the graph, would you say that the...Ch. 2 - How far from the central star does a planet orbit...Ch. 2 - How long does it take a planet to complete one...Ch. 2 - Based on your results from Questions 6 and 7,...Ch. 2 - What is the name of the planet that you identified...Ch. 2 - Using the information provided in the table above...Ch. 2 - A student in your class makes the following...Ch. 2 - Review your answers to Questions 1-4. Do you still...Ch. 2 - Given that Earth is much larger and more massive...Ch. 2 - Prob. 2NEPCh. 2 - How would the strength of the force between the...Ch. 2 - On the diagram, clearly label the location where...Ch. 2 - On the diagram, clearly label the location where...Ch. 2 - Where would the spaceprobe experience the...Ch. 2 - When the spacecraft is at the halfway point, how...Ch. 2 - Two students are discussing their answer to the...Ch. 2 - If the spaceprobe had lost all ability to control...Ch. 2 - Imagine that you need to completely stop the...Ch. 2 - Your weight on Earth is simply the gravitational...Ch. 2 - Which value, apparent magnitude, or absolute...Ch. 2 - Prob. 2APPCh. 2 - Prob. 3APPCh. 2 - Prob. 4APPCh. 2 - The star Lee has an apparent magnitude of 0.1 and...Ch. 2 - Prob. 6APPCh. 2 - Prob. 7APPCh. 2 - Imagine that you are looking at the stars from...Ch. 2 - Repeat Question 1 for July and label the distant...Ch. 2 - In the box below, the same distant stars are shown...Ch. 2 - In the same box, draw another × to indicate the...Ch. 2 - Prob. 5THPCh. 2 - Prob. 6THPCh. 2 - Starting from Earth in January, draw a line...Ch. 2 - Prob. 8THPCh. 2 - Prob. 9THPCh. 2 - Is a parsec a unit of length or a unit of angle?...Ch. 2 - Prob. 11THPCh. 2 - Prob. 12THPCh. 2 - Prob. 13THPCh. 2 - Check your answers to Questions 6 and 11 and...Ch. 2 - What is the angle between you, the house, and the...Ch. 2 - You see the Moon on the horizon just above the...Ch. 2 - Compare your answers for the barn-house angle from...Ch. 2 - Do the angles from above tell you anything about...Ch. 2 - Prob. 5PAPCh. 2 - Prob. 6PAPCh. 2 - Prob. 7PAPCh. 2 - Prob. 8PAPCh. 2 - Prob. 9PAPCh. 2 - Prob. 10PAPCh. 2 - Prob. 11PAPCh. 2 - Prob. 12PAPCh. 2 - Prob. 13PAPCh. 2 - Which object will look brighter from Earth, the...Ch. 2 - Prob. 2SPEPCh. 2 - Star B has an apparent magnitude of 0, which tells...Ch. 2 - Prob. 4SPEPCh. 2 - Prob. 5SPEPCh. 2 - Prob. 6SPEPCh. 2 - Prob. 7SPEP
Additional Science Textbook Solutions
Find more solutions based on key concepts
Choose the best answer to each of the following. Explain your reasoning. One week after full moon, the Moons ph...
The Cosmic Perspective Fundamentals (2nd Edition)
15. In the Olympic shotput event, an athlete throws the shot with an initial speed of 12.0 m/s at a 40.0° angle...
Physics for Scientists and Engineers: A Strategic Approach with Modern Physics (4th Edition)
A locomotive does 7.9 1011 J of work in pulling a 3.4106-kg train 180 km. Find the average force in the couplin...
Essential University Physics: Volume 1 (3rd Edition)
* Elena, a black belt in tae kwon do, is experienced in breaking boards with her fist. A high-speed video indic...
College Physics
Verify that the total number of nucleons, and total charge are conserved for each of the following fusion react...
University Physics Volume 3
A 2000-turn solenoid is 2.0 m long and 15 cm in diameter. The solenoid current is increasing at 1.0 kA/s. (a) F...
Essential University Physics (3rd Edition)
Knowledge Booster
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Similar questions
- Show with a simple diagram how the lower parts of a ship disappear first as it sails away from you on a spherical Earth. Use the same diagram to show why lookouts on old sailing ships could see farther from the masthead than from the deck. Would there be any advantage to posting lookouts on the mast if Earth were flat? (Note that these nautical arguments for a spherical Earth were quite familiar to Columbus and other mariners of his time.)arrow_forwardGalileos telescope showed him that Venus has a large angular diameter (61 arc seconds) when it is a crescent and a small angular diameter (10 arc seconds) when it is nearly full. Use the small-angle formula to find the ratio of its maximum to minimum distance from Earth. Is this ratio compatible with the Ptolemaic universe shown in Figure 3b of the Chapter 4 Concept Art: An Ancient Model of the Universe?arrow_forwardDescribe what an observer at the crater Copernicus would see while the Moon is eclipsed on Earth. What would the same observer see during what would be a total solar eclipse as viewed from Earth?arrow_forward
- What is the difference between asterism d a constellation? Give some examples.arrow_forwardIf you observe light reflected from Saturn’s rings, you should see a redshift at one edge of the rings and a blueshift at the other edge. If you observe a spectral line and see a difference in wavelength of 0.0560 nm between opposite edges of the rings, and the unshifted wavelength (observed in the laboratory) is 500. nm, what is the orbital velocity of particles at the outer edge of the rings? (Hint: Use the Doppler shift formula in Reasoning with Numbers 6-2.)arrow_forwardOn February 28, 2010, Earth was equidistant from the spacecraft Dawn and the Sun, forming an isosceles triangle. The distance from Earth to Dawn and Earth to the Sun was 0.99 AU (astronomical units). The distance from Dawn to the Sun was 1.84 AU. a) Draw a diagram to show Dawn, Earth, and the Sun. b) Determine the angle between the sight lines from Earth to Dawn and the Sun.arrow_forward
- The angle between two lines drawn from a point on Earth to two opposite sides of the Moon make an angle of 0.5 degrees. If you do the same thing for the two opposite ends of Andromeda (as shown above), you find an angle of 5 degrees. Let's assume Andromeda and the Moon are equally far away from our location on Earth (of course that's wrong, but how are we supposed to know?) - then how much larger would the diameter of Andromeda be (as indicated by the arrows at the top), compared to the diameter of the Moon? Pick the answer that's closest to what you get under this hypothetical assumption: A. Equal Diameter B. Twice C. Five times D. Ten timesarrow_forwardWhy are all large celestial bodies (stars, planets, larger moons) very nearly spherical in shape? a because of the centrifugal force from the body's rotation b because of tidal forces c because gravity tries to pull every part of the celestial body to the center d because of the pressure from the heat in the body's corearrow_forwardA solar eclipse is only visible over a narrow strip on the Earth's surface. This is most closely associated with: Select one alternative: The ways in which our view of the sky depends on latitude. The combination of the Earth's rotation on its axis and its movement around the sun. The elliptical nature of the moon's orbit. The perspective dependence associated with parallax. Solar eclipses are actually visible to everyone on the daylight side of the earth.arrow_forward
- The distance light travels in one second(one light-second) is about 1.86×10⁵ mi. Saturn is about 475 light-seconds from the sun. About how many miles from the sun is Saturn?arrow_forwardEarth is about 150 million kilometers from the Sun (1 Astronomical Unit, or AU), and the apparent brightness of the Sun in our sky is about 1300 watts/m2. Using these two facts and the inverse square law for light, determine the apparent brightness that we would measure for the Sun if we were located at the following positions. a) At the orbit of Jupiter (780 million km from the Sun).arrow_forwardWith the aid of a diagram, explain how the Doppler effect can be used to detect the pres- ence of an unseen planet around a nearby star. State how an astronomer can determine if the planet is on a circular or eccentric orbit.arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
- Horizons: Exploring the Universe (MindTap Course ...PhysicsISBN:9781305960961Author:Michael A. Seeds, Dana BackmanPublisher:Cengage LearningStars and GalaxiesPhysicsISBN:9781305120785Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
- AstronomyPhysicsISBN:9781938168284Author:Andrew Fraknoi; David Morrison; Sidney C. WolffPublisher:OpenStaxFoundations of Astronomy (MindTap Course List)PhysicsISBN:9781337399920Author:Michael A. Seeds, Dana BackmanPublisher:Cengage LearningStars and Galaxies (MindTap Course List)PhysicsISBN:9781337399944Author:Michael A. SeedsPublisher:Cengage Learning
Horizons: Exploring the Universe (MindTap Course ...
Physics
ISBN:9781305960961
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Stars and Galaxies
Physics
ISBN:9781305120785
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Foundations of Astronomy (MindTap Course List)
Physics
ISBN:9781337399920
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Stars and Galaxies (MindTap Course List)
Physics
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Cengage Learning
Kepler's Three Laws Explained; Author: PhysicsHigh;https://www.youtube.com/watch?v=kyR6EO_RMKE;License: Standard YouTube License, CC-BY